VLBI of supernovae and gamma-ray bursts

Bietenholz, M. F.

doi:10.22323/1.230.0051

Cited by 1 publication

(2 citation statements)

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“…Taylor et al 2004). Similarly, only ∼30% of the observed core-collapse supernovae were detected in the radio, and only a handful have well-resolved images (Bietenholz 2008(Bietenholz , 2014. The sensitivity of SKA would allow a significantly increased sample of both GRBs and SNe to be resolved with VLBI.…”

Section: Resolving Explosive Outflowsmentioning

confidence: 99%

“…Guirado & Ros 2007;Bower et al 2009). The excellent sensitivity on very long baselines will mean that extragalactic stellar explosions like supernovae (Bietenholz 2008;Perez-Torres et al 2014) and gamma-ray burst afterglows (GRB, Burlon et al 2014, but see also Sect. 7) will be imaged, in total intensity as well as in polarization, in more detail than is possible today.…”

Section: Introductionmentioning

confidence: 99%

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Very Long Baseline Interferometry with the SKA

Zsolt¹,

Leith²,

Cormac³

et al. 2014

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Adding VLBI capability to the SKA arrays will greatly broaden the science of the SKA, and is feasible within the current specifications. SKA-VLBI can be initially implemented by providing phased-array outputs for SKA1-MID and SKA1-SUR and using these extremely sensitive stations with other radio telescopes, and in SKA2 by realising a distributed configuration providing baselines up to thousands of km, merging it with existing VLBI networks. The motivation for and the possible realization of SKA-VLBI is described in this paper.

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Section: Resolving Explosive Outflowsmentioning

confidence: 99%